NGC 2532

NGC 2532 is a barred spiral galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 5,437±13 km/s, which corresponds to a Hubble distance of 261.6 ± 18.3 Mly (80.20 ± 5.62 Mpc). However, seven non-redshift measurements give a much closer mean distance of 128.97 ± 6.85 Mly (39.543 ± 2.099 Mpc). It was discovered by German-British astronomer William Herschel on 5 February 1788.

NGC 2532 has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.